Electronic filter topology

An elementary filter topology introduces a capacitor into the feedback path of an op-amp to achieve an unbalanced active implementation of a low-pass transfer function

Electronic filter topology defines electronic filter circuits without taking note of the values of the components used but only the manner in which those components are connected.

Filter design characterises filter circuits primarily by their transfer function rather than their topology. Transfer functions may be linear or nonlinear. Common types of linear filter transfer function are; high-pass, low-pass, bandpass, band-reject or notch and all-pass. Once the transfer function for a filter is chosen, the particular topology to implement such a prototype filter can be selected so that, for example, one might choose to design a Butterworth filter using the Sallen–Key topology.

Filter topologies may be divided into passive and active types. Passive topologies are comprised exclusively of passive components: resistors, capacitors, and inductors. Active topologies also include active components (such as transistors, op amps, and other Integrated Circuits) that require power. Further, topologies may be implemented either in unbalanced form or else in balanced form when employed in balanced circuits. Implementations such as electronic mixers and stereo sound may require arrays of identical circuits.

Passive topologies

Passive filters have been long in development and use. Most are built from simple two-port networks called "sections". There is no formal definition of a section except that it must have at least one series component and one shunt component. Sections are invariably connected in a "cascade" or "daisy-chain" topology, consisting of either repeats of the same section or of completely different sections. Impedance would combine two sections consisting only of series components or shunt components into a single section.

Some passive filters, consisting of only one or two filter sections, are given special names including the L-section, T-section and Π-section, which are unbalanced filters, and the C-section, H-section and box-section, which are balanced. All are built upon a very simple "ladder" topology (see below). The chart at the bottom of the page shows these various topologies in terms of general constant k filters.

Filters designed using network synthesis usually repeat the simplest form of L-section topology though component values may change in each section. Image designed filters, on the other hand, keep the same basic component values from section to section though the topology may vary and tend to make use of more complex sections.

L-sections are never symmetrical but two L-sections back-to-back form a symmetrical topology and many other sections are symmetrical in form.

Ladder topologies

Ladder topology, often called Cauer topology after Wilhelm Cauer (inventor of the elliptical filter), was in fact first used by George Campbell (inventor of the constant k filter). Campbell published in 1922 but had clearly been using the topology for some time before this. Cauer first picked up on ladders (published 1926) inspired by the work of Foster (1924). There are two forms of basic ladder topologies; unbalanced and balanced. Cauer topology is usually thought of as an unbalanced ladder topology.

A ladder network consists of cascaded asymmetrical L-sections (unbalanced) or C-sections (balanced). In low pass form the topology would consist of series inductors and shunt capacitors. Other bandforms would have an equally simple topology transformed from the lowpass topology. The transformed network will have shunt admittances that are dual networks of the series impedances if they were duals in the starting network - which is the case with series inductors and shunt capacitors.

Image filter sections
 
Unbalanced
L Half section T Section Π Section
Ladder network
 
Balanced
C Half-section H Section Box Section
Ladder network
X Section (mid-T-Derived) X Section (mid-Π-Derived)
N.B. Textbooks and design drawings usually show the unbalanced implementations, but in telecoms it is often required to convert the design to the balanced implementation when used with balanced lines.

Modified ladder topologies

series m-derived topology

Image filter design commonly uses modifications of the basic ladder topology. These topologies, invented by Otto Zobel,[1] have the same passbands as the ladder on which they are based but their transfer functions are modified to improve some parameter such as impedance matching, stopband rejection or passband-to-stopband transition steepness. Usually the design applies some transform to a simple ladder topology: the resulting topology is ladder-like but no longer obeys the rule that shunt admittances are the dual network of series impedances: it invariably becomes more complex with higher component count. Such topologies include;

The m-type (m-derived) filter is by far the most commonly used modified image ladder topology. There are two m-type topologies for each of the basic ladder topologies; the series-derived and shunt-derived topologies. These have identical transfer functions to each other but different image impedances. Where a filter is being designed with more than one passband, the m-type topology will result in a filter where each passband has an analogous frequency-domain response. It is possible to generalise the m-type topology for filters with more than one passband using parameters m1, m2, m3 etc., which are not equal to each other resulting in general mn-type[2] filters which have bandforms that can differ in different parts of the frequency spectrum.

The mm'-type topology can be thought of as a double m-type design. Like the m-type it has the same bandform but offers further improved transfer characteristics. It is, however, a rarely used design due to increased component count and complexity as well as its normally requiring basic ladder and m-type sections in the same filter for impedance matching reasons. It is normally only found in a composite filter.

Bridged-T topologies

Typical bridged-T Zobel network equaliser used to correct high end roll-off

Zobel constant resistance filters[3] use a topology that is somewhat different from other filter types, distinguished by having a constant input resistance at all frequencies and in that they use resistive components in the design of their sections. The higher component and section count of these designs usually limits their use to equalisation applications. Topologies usually associated with constant resistance filters are the bridged-T and its variants, all described in the Zobel network article;

The bridged-T topology is also used in sections intended to produce a signal delay but in this case no resistive components are used in the design.

Lattice topology

Lattice topology X-section phase correction filter

Both the T-section (from ladder topology) and the bridge-T (from Zobel topology) can be transformed into a lattice topology filter section but in both cases this results in high component count and complexity. The most common application of lattice filters (X-sections) is in all-pass filters used for phase equalisation.[4]

Although T and bridged-T sections can always be transformed into X-sections the reverse is not always possible because of the possibility of negative values of inductance and capacitance arising in the transform.

Lattice topology is identical to the more familiar bridge topology, the difference being merely the drawn representation on the page rather than any real difference in topology, cicuitry or function.

Active topologies

Multiple feedback topology

Multiple feedback topology circuit.

Multiple feedback topology is an electronic filter topology which is used to implement an electronic filter by adding two poles to the transfer function. A diagram of the circuit topology for a second order low pass filter is shown in the figure on the right.

The transfer function of the multiple feedback topology circuit, like all second-order linear filters, is:

H(s) = \frac{V_o}{V_i} = -\frac{1}{As^2+Bs+C} = \frac{K {\omega_0}^2}{s^{2}+\frac{\omega_{0}}{Q}s+{\omega_0}^2}.

In an MF filter,

A = (R_1 R_3 C_2 C_5)\,
B = R_3 C_5 + R_1 C_5 + R_1 R_3 C_5/R_4\,
C = R_1/R_4\,
Q = \frac{ \sqrt{R_3 R_4 C_2 C_5} }{ ( R_4 + R_3 + |K| R_3 ) C_5 } is the Q factor.
K = -R_4/R_1\, is the DC voltage gain
\omega_{0} = 2 \pi f_{0} = 1 / \sqrt{R_3 R_4 C_2 C_5} is the corner frequency

Biquad filter

For the digital implementation of a biquad filter, check digital biquad filter.

A biquad filter is a type of linear filter that implements a transfer function that is the ratio of two quadratic functions. The name biquad is short for biquadratic. It is also sometimes called the 'ring of 3' circuit.

Biquad filters are typically active and implemented with a single-amplifier biquad (SAB) or two-integrator-loop topology.

The SAB topology is sensitive to component choice and can be more difficult to adjust. Hence, usually the term biquad refers to the two-integrator-loop state variable filter topology.

Tow-Thomas Biquad Example

For example, the basic configuration in Figure 1 can be used as either a low-pass or bandpass filter depending on where the output signal is taken from.

Figure 1: The common Tow-Thomas biquad filter topology.

The second-order low-pass transfer function is given by

H(s)=\frac{G_\mathrm{lpf}{\omega_0}^2}{s^{2}+\frac{\omega_{0}}{Q}s+{\omega_0}^2}

where low-pass gain G_\mathrm{lpf}=R_{2}/R_{1}. The second-order bandpass transfer function is given by

H(s)=\frac{G_\mathrm{bpf}\frac{\omega_{0}}{Q}s}{s^{2}+\frac{\omega_{0}}{Q}s+{\omega_0}^2}.

with bandpass gain G_\mathrm{bpf}=-R_{3}/R_{1}. In both cases, the

The bandwidth is approximated by B=\omega_{0}/Q, and Q is sometimes expressed as a damping constant \zeta=1/2Q. If a noninverting low-pass filter is required, the output can be taken at the output of the second operational amplifier. If a noninverting bandpass filter is required, the order of the second integrator and the inverter can be switched, and the output taken at the output of the inverter's operational amplifier.

See also

Notes

  1. Zobel, 1923
  2. There is no universally-recognised name for this kind of filter: Zobel (1923, p.11) used the title General Wave-filters having any Pre-assigned Transmitting and Attenuating Bands and Propagation Constants Adjustable Without Changing one Mid-point Characteristic Impedance. Since Zobel refers to the parameters as m1, m2 etc., the shorthand general mn-type seems reasonable terminology to use here.
  3. Zobel, 1928
  4. Zobel, 1931

References

  • Campbell, G A, "Physical Theory of the Electric Wave-Filter", Bell System Technical Journal, November 1922, vol. 1, no. 2, pp. 1–32.
  • Zobel, O J, "Theory and Design of Uniform and Composite Electric Wave Filters", Bell System Technical Journal, Vol. 2 (1923).
  • Foster, R M, "A reactance theorem", Bell System Technical Journal, Vol. 3, pp. 259–267, 1924.
  • Cauer, W, "Die Verwirklichung der Wechselstromwiderstande vorgeschriebener Frequenzabhängigkeit", Archiv für Elektrotechnik, 17, pp. 355–388, 1926.
  • Zobel, O J, "Distortion correction in electrical networks with constant resistance recurrent networks", Bell System Technical Journal, Vol. 7 (1928), p. 438.
  • Zobel, O J, Phase-shifting network, US patent 1 792 523, filed 12 March 1927, issued 17 Feb 1931.